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Geant4 Simulations for the Radon Electric Dipole Moment Search at

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distribution, this average intensity can increase or decrease over <strong>the</strong> depolariz<strong>at</strong>ion<br />

time. The 416 keV M1 transition shown in Figure 4.5(b) clearly illustr<strong>at</strong>es this effect.<br />

Even though <strong>the</strong> number of nuclei inside <strong>the</strong> cell, and hence <strong>the</strong> total activity is<br />

decreasing, <strong>the</strong> observed average count r<strong>at</strong>e increases over <strong>the</strong> depolariz<strong>at</strong>ion time<br />

scale (which is short compared to <strong>the</strong> 223 Rn half-life of 24.3 minutes). This change<br />

in <strong>the</strong> average count r<strong>at</strong>e occurs because <strong>the</strong> “donut shaped” distribution depolarizes<br />

into an isotropic distribution th<strong>at</strong> has a larger average γ-ray intensity in <strong>the</strong> plane of<br />

<strong>the</strong> eight GRIFFIN detectors. This effect is fur<strong>the</strong>r studied in Figures 4.6 and 4.7.<br />

The remaining terms describe <strong>the</strong> precession, where A 5 is <strong>the</strong> frequency, A 6 is <strong>the</strong><br />

phase and A 7 , A 8 , A 9 , ··· are <strong>the</strong> intensities of odd-sine oscill<strong>at</strong>ions. A maximum of<br />

14 odd-sine terms were included into <strong>the</strong> fitting program (up to A 20 ), however, often<br />

only <strong>the</strong> first few odd-sine terms were non-zero. In this case all o<strong>the</strong>r sine terms fixed<br />

to zero and removed from <strong>the</strong> fit.<br />

Figure 4.8 illustr<strong>at</strong>es <strong>the</strong> fit to <strong>the</strong> 416 keV time projection d<strong>at</strong>a given in Figure<br />

4.5(b). In <strong>the</strong> fit <strong>the</strong> half-life was “fixed” to its simul<strong>at</strong>ed value of 1458 seconds<br />

and <strong>the</strong> remaining parameters were left “free” to be fitted by <strong>the</strong> program. The fit<br />

resulted in a good reduced χ 2 of 1.04 and a precession frequency which agrees with<br />

<strong>the</strong> simul<strong>at</strong>ed value of 2 Hz. The input precession frequency was 1 Hz, but due to <strong>the</strong><br />

symmetric n<strong>at</strong>ure of <strong>the</strong> γ-ray angular distribution <strong>the</strong> observed frequency is twice<br />

<strong>the</strong> input value. The fitted parameters are summarized in Table 4.1. It should be<br />

noted th<strong>at</strong> <strong>the</strong> analyzing power A in Equ<strong>at</strong>ion 4.1, which th<strong>at</strong> detects a change of<br />

counts ∆N = AN, was estim<strong>at</strong>ed as A = 0.2 in <strong>the</strong> calcul<strong>at</strong>ed st<strong>at</strong>istical limits <strong>for</strong><br />

<strong>the</strong> RnEDM experiment [32]. Figure 4.8 valid<strong>at</strong>es th<strong>at</strong> estim<strong>at</strong>e as <strong>the</strong> r<strong>at</strong>io of <strong>the</strong><br />

signal amplitude to <strong>the</strong> background is approxim<strong>at</strong>ely 0.2.<br />

From this single measurement we can calcul<strong>at</strong>e <strong>the</strong> resulting sensitivity in <strong>the</strong><br />

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